SDO HMI 2011-07-16 13:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 43.84 | 283.55 | 22.61 | 146.44 | 16.50 | 169.22 | -11.19 | 41.47 | 0.2822 | -753.9 | -397.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.36 | 273.74 | 0.19 | 141.21 | 16.80 | 169.48 | -10.94 | 40.12 | 0.2831 | -973.0 | -433.0 | |
| 32.68 | -1.00 | 16.85 | -1.00 | 16.42 | 169.40 | -11.01 | 41.22 | 0.2793 | -1259.8 | 999999 | |
| 1.54 | -1.00 | 0.80 | -1.00 | 16.77 | 169.35 | -11.06 | 40.52 | 0.2841 | -966.1 | 999999 | |
| 7.26 | -1.00 | 3.74 | -1.00 | 15.99 | 169.36 | -11.05 | 42.41 | 0.2744 | -1307.7 | 999999 | |
| 2.00 | -1.00 | 1.03 | -1.00 | 16.14 | 168.93 | -11.48 | 43.09 | 0.2811 | -830.0 | 999999 | |
| 0.00 | 0.82 | 0.00 | 0.42 | 16.15 | 168.03 | -12.39 | 45.16 | 0.2919 | -685.0 | -468.6 | |
| 0.00 | 1.27 | 0.00 | 0.66 | 16.39 | 167.16 | -13.25 | 46.43 | 0.3048 | -760.0 | -567.8 | |
| 0.00 | 0.91 | 0.00 | 0.48 | 20.97 | 166.59 | -13.82 | 37.88 | 0.3649 | 815.0 | 615.5 | |
| 0.00 | 1.09 | 0.00 | 0.58 | 21.09 | 166.14 | -14.27 | 38.52 | 0.3709 | 831.0 | 726.4 | |
| 0.00 | 1.36 | 0.00 | 0.73 | 20.96 | 166.12 | -14.29 | 38.79 | 0.3696 | 937.0 | 693.7 | |
| 0.00 | 1.09 | 0.00 | 0.57 | 15.97 | 164.77 | -15.64 | 51.97 | 0.3306 | 797.0 | 593.8 | |
| 0.00 | 1.45 | 0.00 | 0.79 | 23.77 | 163.85 | -16.56 | 37.98 | 0.4257 | 868.0 | 612.0 | |
| 0.00 | 0.73 | 0.00 | 0.39 | 19.51 | 163.27 | -17.15 | 46.53 | 0.3845 | 790.0 | 694.0 | |
| 0.00 | 1.09 | 0.00 | 0.61 | 23.04 | 160.07 | -20.35 | 44.68 | 0.4569 | 726.0 | 604.2 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
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that the umbra consists of fragmented regions which cannot be separated without losing umbral area. In this way several spots (intensity minima in the umbra) have a common umbra, e.g. -2 means that the given spot shares an umbra with spot No.2, and the common U value is indicated at spot No.2. |
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| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
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that several umbras have a common penumbra, e.g. -7 means that the given umbra shares a penumbra with umbra No.7, and the WS value is indicated at No.7. |
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| Corr. U | - Corrected umbra area in millionths of solar hemisphere, for negative values see above | |
| Corr. WS | - Corrected whole spot area in millionths of solar hemisphere, for negative values see above | |
| B | - Heliographic latitude B; positive: North, negative: South | |
| L | - Heliographic longitude L | |
| LCM | - Longitudinal distance from the Sun's central meridian | |
| Pos. angle | - Position angle | |
| r | - Distance from the centre of Sun's disc in terms of Sun's radius | |
| MU | - Mean magnetic field within the umbra contour averaged the pixel values with sign. | |
| MP | - Mean magnetic field within the penumbra contour averaged the pixel values with sign. | |